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PDF (Chapter 3) 44 Chapter 3: Subduction Transition and Flat Slab Structure of the Subduction Transition Region from Seismic Array Data in Southern Peru Kristin Phillips and Robert W. Clayton Abstract Data from three seismic arrays installed in southern Peru was analyzed using receiver functions from P, PP, and PKP wave phases, in order to image the subducted Nazca slab. The arrays cover the transition region from flat slab subduction in central Peru to normal subduction with an angle of about 30˚ further south. The results provide an image of the flattened slab from the coast to approximately 300 km inland and also across the transition region from flat to 30-degree subduction, which appears to be a bend rather than a tear in the slab. In the flat slab region, the slab is well defined near the coast and flattens out at 100 km depth beneath the Altiplano. The slab appears to start flattening some 400 km in advance of the subduction of the Nazca Ridge and the flattening is maintained for 1300 km after its passage. The Moho begins at a depth of around 30 km near the coast and has a maximum depth of 75 km beneath the Altiplano, consistent with the results of the other arrays. The Vp/Vs ratios for both arrays exhibit average values between 1.73 and 1.75 indicating that the region is most likely not actively volcanic. The images also show a positive-impedance midcrustal structure at 45 around 40 km depth, which is suggested to be a result of underthrusting of the Brazilian shield. This would explain the missing crust needed to support the Altiplano. 3.1. Introduction The dip of the subducted Nazca plate beneath southern Peru changes from shallow or flat slab beneath central Peru to a steeper dip angle (“normal” subduction) of around 30 degrees beneath southern Peru. This transition is evident in the seismicity (Barazangi & Isacks, 1976; Cahill and Isacks, 1992; Grange et al, 1984; Suarez et al, 1983), and by a gap in the arc-volcanism (Gutsher, Olivet et al, 1999; Gutscher, Spakman et al. 2000; McGeary et al, 1985). Adakitic magmas have also been associated with flat slab regions (Gutscher, Maury, et al. 2000) and have been reported in southern Ecuador/northern Peru (Beate et al, 2001). They are suggested to result from partial melting of subducted oceanic crust (Gutscher, Maury, et al. 2000). Besides the observed correspondence between adakites and flat slab regions, the partial melting resulting in such magmas could also be a result of slab tearing at the transitions from flat slab to a steeper dip angle (Yogodzinski et al, 2001). The lack of reported adakites in southern Peru might indicate that the southern transition is slab bending rather than a tear. The change in dip is coincident with the subduction of Nazca Ridge. This is one of three zones of slab-dip changes along the western margin of Southern America. In central Chile, the subduction of the Juan Fernandez Ridge is cited as the cause of the flattening along its subduction trajectory (Pilger, 1981; Gutscher, Spakman et al, 2000; von Huene et al, 1997), and the study of Anderson et al (2007) show that the zone of 46 flattening tightly conforms to the shape of the ridge. In Equador, the Carnegie Ridge also apparently causes the slab to flatten (Gutscher,Malavielle et al. 1999). Various mechanisms have been proposed as to the cause of flat slab subduction. Some authors have noted a correlation between regions of flat slab subduction and the presence of thickened oceanic crust such as that due to a subducting plateau or ridge which could increase the buoyancy of the subducting slab (Gutscher, Maury et al. 2000). Gutscher et al. (1999) proposed that the length of flat subduction in Peru was due to buoyancy effects resulting from two subducting ridges; the Nazca ridge and a previously unknown impactor referred to as the Inca Plateau which is believed to be the mirror image of the Marquesas plateau although recent plate movement reconstructions call into question the proposed location and timing of the Inca plateau (Skinner and Clayton 2012). Both plateaus were suggested to have formed at the Pacific-Farallon spreading centre based on tectonic reconstructions. According to Hampel (2002), the Nazca Ridge originally began subducting at 11˚S around 11.2 Ma. Since then it has been sweeping south and presently has a migration rate of around 43 cm per year. The area of flat subduction in Peru corresponds to the area swept out by the Nazca Ridge. Thus the Nazca Ridge may have had an impact on the evolution and shape of the subduction zone. In addition to buoyancy effects caused by a subducting ridge or plateau, other factors could influence flat subduction such as the age of the lithosphere being subducted (Sacks 1983), delay in the basalt to eclogite transformation (Gutscher, Spakman et al. 2000; Pennington 1984), absolute motion of the upper plate (Olbertz et al. 1997), the convex curvature of the Peruvian margin (Bevis, 1986; Cahill and Isacks, 47 1992), intraplate hydrostatic suction (Jischke, 1975), or cycles of flat subduction caused by rebound after a steepening slab breaks off (Haschke et al, 2002). Modeling has been done in several studies to address the relative importance of different causes for flat slab subduction. Van Hunen et al (2002a) suggested that relative motion of the upper plate could be equally or more important than plateau subduction based on numerical studies; however this is a factor that is present in the region of normal subduction as well. The dominant mechanism for flat slab subduction needs to be considered independently for each subduction zone since some factors are present in both normal and flat slab regions, while other factors can be observed in only some flat slab regions and not in others. One of the puzzling aspects of the flat subduction in southern Peru is the fact that the slab does not return to a normal dip angle after the impactor has passed. This contrasts with central Chile where the slab returns to normal dip at a distance of about 150 km on either side of the track of the JFR (based on contours from Anderson et al, 2007). In this study, we examine the details of the transition zone between normal and flat subduction using dense seismic arrays, which include instruments both in the flat-slab zone as well as an array parallel to the trench to sample the subduction transition. The array in the flat slab region near the Nazca Ridge provides an opportunity to study the effect of the Nazca Ridge on the subduction zone in Southern Peru. A previous study (Phillips et al, 2012) has described the results of a line (Line 1, figure 3.1) that is in the normal-dip part of the zone. It succeeded in imaging the slab down to 250 km, and found a midcrustal velocity increase at about 40 km depth suggested to be 48 underthrusting by the Brazilian shield. In this study we expand on those results by presenting details of the transition and flat slab subduction regions. Receiver function studies performed here provide details of the structure of the subduction system including Moho depth and shape of the slab as well as velocity information such as Vp/Vs ratio. Corresponding images show the transition from normal to flat slab subduction and the shape of the slab in the flat slab region, which is affected by the subducting Nazca Ridge. The structure of the flat slab region is compared to the study of the normal subduction regime. Figure 3.1. Location of the seismic arrays in Southern Peru as denoted by red circles. Added stations from the PULSE and CAUGHT experiments are shown as orange and purple circles respectively. The topography and bathymetry shows the incoming Nazca 49 Ridge and the Altiplano of the Andes. Slab contours are based on fits to seismicity and comes from the Slab 1.0 model (Hayes et al, 2012). Active and dormant volcanoes are denoted by white and blue triangles. The three seismic arrays are labeled “Line 1,” “Line 2,” and “Line 3.” Line 1 is located in the region of normal subduction, Line 2 samples the transition from normal to flat slab subduction, and Line 3 is in the flat slab region. The black lines along Lines 2 and 3 with endpoints labeled A, B, and C correspond to cross section profiles in figure 3.2. 3.2. Methods 3.2.1 Stations and Data Three lines of broadband sensors were installed as part of the Peru Subduction Experiment (PeruSE) as seen in figure 3.1. The first line (Line 1) deployed perpendicular to the trench from Mollendo on the coast to Juliaca near Lake Titicaca, samples the region of normal subduction dip (Phillips et al, 2012). The second seismic array (Line 2) runs parallel to the trench from Juliaca to Cusco sampling the transitional region where the subduction regime changes to shallow subduction. It includes 50 broadband seismic stations over a distance of about 300 km resulting in an average station spacing of about 6 kilometers. Line 3 is perpendicular to the trench starting on the coast near the city of Nazca and runs inland through Cusco for 509 km. It consists of 40 stations from the PeruSE network plus 5 stations from the PULSE network (Eakin et al, 2011). Line 3 is located near where the Nazca Ridge is subducting beneath South America and samples the flat slab region. In addition, 2 stations from the CAUGHT network (Ryan et al, 2011) that are in the interior of the box defined by the networks described above are used.
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